Never bet against Einstein

Abstract

Among the geniuses of mankind, Einstein was probably one of those who made more erroneous claims, and often changed his opinion during the years on important scientific subjects. However, it is important to bear in mind that his mistakes were always due to a misinterpretation of the results obtained from his equations, since he was often biased by his own view of the universe. Einstein's equations have always given the correct answer and, till now, there is no evidence that they might not be correct.

arXiv comment19 pages; in press on IJMPD. arXiv admin note: text overlap with arXiv:1602.04674 by other author

References in corpus (82)

• Observation of Gravitational Waves from a Binary Black Hole Merger
• The Confrontation between General Relativity and Experiment
• A Massive Pulsar in a Compact Relativistic Binary
• Multi-messenger Observations of a Binary Neutron Star Merger
• Closest Star Seen Orbiting the Supermassive Black Hole at the Centre of the Milky Way
• Viewing the Shadow of the Black Hole at the Galactic Center
• An increased estimate of the merger rate of double neutron stars from observations of a highly relativistic system
• Stellar Orbits Around the Galactic Center Black Hole
• The NANOGrav 12.5-year Data Set: Search For An Isotropic Stochastic Gravitational-Wave Background
• Possible Gravitational Microlensing of a Star in the Large Magellanic Cloud
• The First Measurement of Spectral Lines in a Short-Period Star Bound to the Galaxy's Central Black Hole: A Paradox of Youth
• Gravitational lensing in the strong field limit
• SINFONI in the Galactic Center: young stars and IR flares in the central light month
• Binary and Millisecond Pulsars
• Microlensing constraints on primordial black holes with the Subaru/HSC Andromeda observation
• Real-Time Difference Imaging Analysis of MOA Galactic Bulge Observations During 2000
• Unbound or Distant Planetary Mass Population Detected by Gravitational Microlensing
• An Update on Monitoring Stellar Orbits in the Galactic Center
• The International Pulsar Timing Array: First Data Release
• Strong field limit of black hole gravitational lensing
• Gravitational wave bursts from cusps and kinks on cosmic strings
• Candidate Electromagnetic Counterpart to the Binary Black Hole Merger Gravitational Wave Event S190521g
• Wave Effects in Gravitational Lensing of Gravitational Waves from Chirping Binaries
• Gravitational Test Beyond the First Post-Newtonian Order with the Shadow of the M87 Black Hole
• On the evidence for a common-spectrum process in the search for the nanohertz gravitational-wave background with the Parkes Pulsar Timing Array
• Confirmation of general relativity on large scales from weak lensing and galaxy velocities
• One Channel to Rule Them All? Constraining the Origins of Binary Black Holes using Multiple Formation Pathways
• Ultra-Low Frequency Gravitational Radiation from Massive Black Hole Binaries
• Has NANOGrav found first evidence for cosmic strings?
• Relativistic Measurements from Timing the Binary Pulsar PSR B1913+16
• A Multi-Mass Velocity Dispersion Model of 47 Tucanae Indicates No Evidence for an Intermediate Mass Black Hole
• A precise extragalactic test of General Relativity
• Relativistic deflection of background starlight measures the mass of a nearby white dwarf star
• Mirages around Kerr black holes and retro-gravitational lenses
• Light curves of light rays passing through a wormhole
• ExELS: an exoplanet legacy science proposal for the ESA Euclid mission I. Cold exoplanets
• On the core-halo distribution of dark matter in galaxies
• Direct Measurements of Black Hole Charge with Future Astrometrical Missions
• Precision Gravity Tests and the Einstein Equivalence Principle
• Direct limits for scalar field dark matter from a gravitational-wave detector
• Gravitational Lensing by Black Holes: a comprehensive treatment and the case of the star S2
• Second-generation microlensing planet surveys: a realistic simulation
• Pixel-lensing as a way to detect extrasolar planets in M31
• A terrestrial-mass rogue planet candidate detected in the shortest-timescale microlensing event
• The Anomaly in the Candidate Microlensing Event PA-99-N2
• Gravitational wave energy emission and detection rates of Primordial Black Hole hyperbolic encounters
• First Resolution of Microlensed Images
• Retro-MACHOs: Pi in the sky?
• Retrolensing by a wormhole at deflection angles $\pi$ and $3\pi$
• Gravitational wave energy spectrum of hyperbolic encounters
• Sgr A${}^{\ast }$: a laboratory to measure the central black hole and cluster parameters
• First Microlensing Events From The MEGA Survey Of M31
• Gravitational waves from hyperbolic encounters
• Noise analysis in the European Pulsar Timing Array data release 2 and its implications on the gravitational-wave background search
• The galactic center black hole as a possible retro-lens for the S2 orbiting star
• Gravitational Wave observatories may be able to detect hyperbolic encounters of Black Holes
• Estimating the parameters of the Sgr A* black hole
• WFIRST Planet Masses from Microlens Parallax
• Gravitational wave propagation beyond geometric optics
• Photometric, Astrometric and Polarimetric observations of gravitational microlensing events
• Discovery of a bright microlensing event with planetary features towards the Taurus region: a super Earth planet
• Estimating Finite Source Effects in Microlensing Events due to Free-Floating Planets with the Euclid Survey
• Astrometric Properties of Gravitational Binary-Microlens Events and Their Applications
• Astrometric Microlensing as a Method of Discovering and Characterizing Extra-Solar Planets
• Kerr black holes as retro-MACHOs
• Search for exoplanets in M31 with pixel-lensing and the PA-99-N2 event revisited
• WFIRST and EUCLID: enabling the microlensing parallax measurement from space
• A note on gravitational wave lensing
• Signatures of rotating binaries in micro-lensing experiments
• Principles of Gravitational-Wave Detection with Pulsar Timing Arrays
• Astrophysical implications of gravitational microlensing of gravitational waves
• The Wendelstein Calar Alto Pixellensing Project (WeCAPP): the M31 Nova catalogue
• A Quasar microlensing event towards J1249+3449?
• The Scales of Gravitational Lensing
• Trajectories of the images in binary microlensing
• Astrometric microlensing
• Parallax and orbital effects in astrometric microlensing with binary sources
• M31 Pixel Lensing PLAN Campaign: MACHO Lensing and Self Lensing Signals
• Starspot induced effects in microlensing events with rotating source star
• Timing analysis in microlensing
• Investigating the free-floating planet mass by Euclid observations
• Gravitational wave scintillation by a stellar cluster

Cited by in corpus (2)

• Shadows near supermassive black holes: from a theoretical concept to GR test
• Description and Application of the Surfing Effect